English

Polarized Cosmological Gravitational Waves from Primordial Helical Turbulence

Astrophysics 2015-06-24 v2 General Relativity and Quantum Cosmology Chaotic Dynamics Fluid Dynamics

Abstract

We show that helical turbulence produced during a first-order phase transition generates circularly polarized cosmological gravitational waves (GWs). The characteristic frequency of these GWs for an extreme case of the phase transition model is around 10310^{-3} --- 10210^{-2} Hz with an energy density parameter as high as 101210^{-12} --- 101110^{-11}. The possibility of detection is briefly discussed.

Keywords

Cite

@article{arxiv.astro-ph/0505628,
  title  = {Polarized Cosmological Gravitational Waves from Primordial Helical Turbulence},
  author = {Tina Kahniashvili and Grigol Gogoberidze and Bharat Ratra and ;},
  journal= {arXiv preprint arXiv:astro-ph/0505628},
  year   = {2015}
}

Comments

4 pages, 1 figure, references added, Phys. Rev. Lett. in press